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- W2060645712 abstract "Models of secluded dark matter offer a variant on the standard WIMP picture and can modify our expectations for hidden sector phenomenology and detection. In this work we extend a minimal model of secluded dark matter, comprised of a U(1)'-charged dark matter candidate, to include a confining hidden-sector CFT. This provides a technically natural explanation for the hierarchically small mediator-scale, with hidden-sector confinement generating m_{gamma'}>0. Furthermore, the thermal history of the universe can differ markedly from the WIMP picture due to (i) new annihilation channels, (ii) a (potentially) large number of hidden-sector degrees of freedom, and (iii) a hidden-sector phase transition at temperatures T << M_{dm} after freeze out. The mediator allows both the dark matter and the Standard Model to communicate with the CFT, thus modifying the low-energy phenomenology and cosmic-ray signals from the secluded sector." @default.
- W2060645712 created "2016-06-24" @default.
- W2060645712 creator A5013846393 @default.
- W2060645712 creator A5038190840 @default.
- W2060645712 date "2012-08-01" @default.
- W2060645712 modified "2023-09-27" @default.
- W2060645712 title "Secluded dark matter coupled to a hidden CFT" @default.
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- W2060645712 doi "https://doi.org/10.1007/jhep08(2012)048" @default.
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